arXiv · 1405.1862
Translation invariant time-dependent solutions to massive gravity II
Abstract
This paper is a sequel to arXiv:1310.6560 [hep-th] and is also devoted to translation-invariant solutions of ghost-free massive gravity in its moving frame formulation. Here we consider a mass term which is linear in the vielbein (corresponding to a $β_3$ term in the 4D metric formulation) in addition to the cosmological constant. We determine explicitly the constraints, and from the initial value formulation show that the time-dependent solutions can have singularities at a finite time. Although the constraints give, as in the $β_1$ case, the correct number of degrees of freedom for a massive spin two field, we show that the lapse function can change sign at a finite time causing a singular time evolution. This is very different to the $β_1$ case where time evolution is always well defined. We conclude that the $β_3$ mass term can be pathological and should be treated with care.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
J. Mourad, D. A. Steer. 2014-05-08. Translation invariant time-dependent solutions to massive gravity II. https://doi.org/10.1088/1475-7516%2F2014%2F06%2F058
Cite the original work for its findings. Save a collection to share your selection of sources.